On the Nature of an Anomalously Slow Apsidal Motion of Di-Herculis

Details On the Nature of an Anomalously Slow Apsidal Motion of Di-Herculis On the Nature of an Anomalously Slow Apsidal Motion of Di-Herculis

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988atsir1529...13z&link_type=abstract

Astronomicheskii Tsirkulyar NO.1529/JUN, P.13, 1988

Astronomy and Astrophysics

Astronomy

2

Scientific paper

A three-body model of the eclipsing system DI Her is proposed to explain
the anomalously slow apsidal motion. The influence of the third body,
whose orbit is close to the visual plane, results in significant
decrease of the binary system's eccentricity.

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